Plasma Wave Evidence for Lightning on Venus

Robert J. Strangeway

Institute of Geophysics and Planetary Physics, University of California at Los Angeles

J. Atmos. Terr. Phys., 57, 537-556, 1995
(Received in final form 19 May 1994; accepted 27 June 1994)
Copyright © 1995, Elsevier Science Ltd


      Plasma wave data from the Pioneer Venus Orbiter provide the largest body of data cited as evidence for lightning on Venus. These data are also the most controversial, mainly because of the ambiguity in mode identification due to limited spectral information. We review some of the more recent studies of the plasma wave data at Venus, and we demonstrate that the characteristics of the 100 Hz waves are consistent with whistler-mode waves propagating vertically from below the ionosphere. We further show that in situ instabilities are too weak to generate whistler-mode waves, mainly because the thermal pressure is comparable to the magnetic field pressure in the ionosphere of Venus. The lower hybrid drift instability has also been suggested as an alternative source for the 100 Hz waves. However, the wave properties are more consistent with whistler-mode propagation; the lower hybrid drift instability requires very short gradient scale lengths to overcome damping due to collisions. We also note that an apparent association between Langmuir probe anomalies and 100 Hz waves is much lower than previously reported, once we apply a consistent intensity threshold for identifying wave bursts. The lightning hypothesis remains the most probable explanation of the plasma waves detected at low altitudes in the nightside ionosphere of Venus.


      1. Introduction
      2. The Morphology of the VLF/ELF Bursts
      3. Lightning or Whistler-Mode Instability
      4. Lightning or Density Fluctuations
      5. Lightning or Lower Hybrid Instability
      6. Conclusions
      Figure Captions

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